Feynman's i-epsilon prescription, almost real spacetimes, and acceptable complex spacetimes
Matt Visser (Victoria University of Wellington)

TL;DR
This paper reinterprets Feynman's i-epsilon prescription as a complex deformation of spacetime metrics, extending it to curved and fluctuating geometries, and explores constraints on acceptable complex metrics for quantum gravity.
Contribution
It introduces a novel interpretation of the i-epsilon prescription as a complex metric deformation, connecting it to acceptable complex metrics and quantum gravity path integrals.
Findings
Reinterpretation of i-epsilon as complex metric deformation
Extension to semi-classical curved spacetimes and fluctuating geometries
Explicit construction of acceptable complex metrics in tetrad formalism
Abstract
Feynman's i-epsilon prescription for quantum field theoretic propagators has a quite natural reinterpretation in terms of a slight complex deformation of the Minkowski spacetime metric. Though originally a strictly flat-space result, once reinterpreted in this way, these ideas can be naturally extended first to semi-classical curved-spacetime QFT on a fixed background geometry and then, (with more work), to fluctuating spacetime geometries. There are intimate connections with variants of the weak energy condition. We shall take the Lorentzian signature metric as primary, but note that allowing the complex deformation to become large leads to a variant of Wick rotation, and more importantly leads to physically motivated constraints on the configuration space of acceptable off-shell geometries to include in Feynman's functional integral when attempting to quantize gravity. Ultimately this…
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Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics
